Early views of the Martian surface from the Mars orbiter camera of Mars global surveyor

被引:191
作者
Malin, MC
Carr, MH
Danielson, GE
Davies, ME
Hartmann, WK
Ingersoll, AP
James, PB
Masursky, H
McEwen, AS
Soderblom, LA
Thomas, P
Veverka, J
Caplinger, MA
Ravine, MA
Soulanille, TA
机构
[1] Malin Space Sci Syst, San Diego, CA 92191 USA
[2] US Geol Survey, Menlo Park, CA 94025 USA
[3] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[4] Rand Corp, Santa Monica, CA 90406 USA
[5] Planetary Sci Inst, Tucson, AZ 85719 USA
[6] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA
[7] US Geol Survey, Flagstaff, AZ 86001 USA
[8] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[9] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA
[10] Prama Corp, Pasadena, CA 91116 USA
关键词
D O I
10.1126/science.279.5357.1681
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
High-resolution images of the martian surface at scales of a few meters show ubiquitous erosional and depositional eolian landforms. Dunes, sandsheets, and drifts are prevalent and exhibit a range of morphology, composition (inferred from albedo), and age (as seen in occurrences of different dune orientations at the same location). Steep walls of topographic depressions such as canyons, valleys, and impact craters show the martian crust to be stratified at scales of a few tens of meters. The south polar layered terrain and superposed permanent ice cap display diverse surface textures that may reflect the complex interplay of volatile and non-volatile components, Low resolution regional views of the planet provide synoptic observations of polar cap retreat, condensate clouds, and the lifecycle of local and regional dust storms.
引用
收藏
页码:1681 / 1685
页数:5
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